The Milky Way
The Milky Way, photographed by R. Scott Hinks from Sydney, Australia
The Milky Way is the galaxy in which the Sun lies. It is estimated to contain around 200 billion stars, in a flat disk-like structure.
The Sun lies about two-thirds of the way out from the centre of the disk, at a distance of around 8 kiloparsec. The chart below shows an approximate cross-section through the galaxy, with the position of the Sun marked. The grey region marks the disk of the galaxy, where most of the stars and open star clusters lie. The dots show the approximate distribution of larger globular star clusters, which form a spherical halo around the center of the galaxy.
The distribution of deep sky objects
Because we lie within the disk of the galaxy, it appears as a band of light which encircles the entire sky.
The chart below shows the distribution of various kinds of deep sky object across the night sky. The blue dots represent open star clusters, which are heavily concentrated in the plane of the galaxy. The green dots represent globular star clusters, which are seen all around the sky, but concentrate particularly around the constellation Sagittarius, at a right ascension of around 18 hours. This is the direction in which the center of the galaxy lies.
The red dots show external galaxies, which are more distant. They tend to be seen predominantly away from the plane of the Milky Way. This has nothing to do with their physical distribution in space, but is merely because it is harder to see galaxies which lie behind the plane of the Milky Way, as there is too much material in the way.
An approximate model of the Milky Way's spiral arms
The chart below shows an approximate map of the Milky Way's spiral arms.